Physics:Isotopes of unbinilium

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Short description: Nuclides with atomic number of 120 but with different mass numbers

Unbinilium (120Ubn) has not yet been synthesised, so all data would be theoretical and a standard atomic weight cannot be given. Like all synthetic elements, it would have no stable isotopes.

List of isotopes

No isotopes of unbinilium are known.

Nucleosynthesis

Target-projectile combinations leading to Z = 120 compound nuclei

The below table contains various combinations of targets and projectiles that could be used to form compound nuclei with Z=120.[1]

Target Projectile CN Attempt result
208Pb 88Sr 296Ubn Reaction yet to be attempted
238U 64Ni 302Ubn Failure to date
237Np 59Co 296Ubn Reaction yet to be attempted
244Pu 58Fe 302Ubn Failure to date
244Pu 60Fe 304Ubn Reaction yet to be attempted
243Am 55Mn 298Ubn Reaction yet to be attempted
245Cm 54Cr 299Ubn[2] Reaction yet to be attempted
248Cm 54Cr 302Ubn Failure to date
250Cm 54Cr 304Ubn Reaction yet to be attempted
249Bk 51V 300Ubn Reaction yet to be attempted
249Cf 50Ti 299Ubn Failure to date
250Cf 50Ti 300Ubn Reaction yet to be attempted
251Cf 50Ti 301Ubn Reaction yet to be attempted
252Cf 50Ti 302Ubn Reaction yet to be attempted
257Fm 48Ca 305Ubn Reaction yet to be attempted

Hot fusion

238U(64Ni,xn)302-xUbn

In April 2007, the team at the GSI Helmholtz Centre for Heavy Ion Research in Darmstadt, Germany attempted to create unbinilium using a 238U target and a 64Ni beam:[3]

23892U + 6428Ni → 302120Ubn* → no atoms

No atoms were detected, providing a limit of 1.6 pb for the cross section at the energy provided. The GSI repeated the experiment with higher sensitivity in three separate runs in April–May 2007, January–March 2008, and September–October 2008, all with negative results, reaching a cross section limit of 90 fb.[3]

244Pu(58Fe,xn)302-xUbn

Following their success in obtaining oganesson by the reaction between 249Cf and 48Ca in 2006, the team at the Joint Institute for Nuclear Research (JINR) in Dubna started experiments in March–April 2007 to attempt to create unbinilium with a 58Fe beam and a 244Pu target.[4][5] Initial analysis revealed that no atoms of unbinilium were produced, providing a limit of 400 fb for the cross section at the energy studied.[6]

24494Pu + 5826Fe → 302120Ubn* → no atoms

The Russian team planned to upgrade their facilities before attempting the reaction again.[6]

245Cm(54Cr,xn)299-xUbn

There are indications that this reaction may be tried by the JINR in future. The expected products of the 3n and 4n channels, 296120 and 295120, could undergo five alpha decays to reach the darmstadtium isotopes 276Ds and 275Ds respectively; these darmstadtium isotopes were synthesised at the JINR in 2022 and 2023 respectively, both in the 232Th+48Ca reaction.[2][7]

248Cm(54Cr,xn)302-xUbn

In 2011, after upgrading their equipment to allow the use of more radioactive targets, scientists at the GSI attempted the rather asymmetrical fusion reaction:[8]

24896Cm + 5424Cr → 302120Ubn* → no atoms

It was expected that the change in reaction would quintuple the probability of synthesizing unbinilium,[9] as the yield of such reactions is strongly dependent on their asymmetry.[10] Although this reaction is less asymmetric than the 249Cf+50Ti reaction, it also creates more neutron-rich unbinilium isotopes that should receive increased stability from their proximity to the shell closure at N = 184.[11] Three signals were observed in May 2011; a possible assignment to 299Ubn and its daughters was considered,[12] but could not be confirmed,[13][14][11] and a different analysis suggested that what was observed was simply a random sequence of events.[15]

In March 2022, Yuri Oganessian gave a seminar at the JINR considering how one could synthesise element 120 in the 248Cm+54Cr reaction.[16] In 2023, the director of the JINR, Grigory Trubnikov, stated that he hoped that the experiments to synthesise element 120 will begin in 2025.[17]

249Cf(50Ti,xn)299-xUbn

In August–October 2011, a different team at the GSI using the TASCA facility tried a new, even more asymmetrical reaction:[8][18]

24998Cf + 5022Ti → 299120Ubn* → no atoms

Because of its asymmetry,[19] the reaction between 249Cf and 50Ti was predicted to be the most favorable practical reaction for synthesizing unbinilium, although it is also somewhat cold, and is further away from the neutron shell closure at N = 184 than any of the other three reactions attempted. No unbinilium atoms were identified, implying a limiting cross section of 200 fb.[18] Jens Volker Kratz predicted the actual maximum cross section for producing unbinilium by any of the four reactions 238U+64Ni, 244Pu+58Fe, 248Cm+54Cr, or 249Cf+50Ti to be around 0.1 fb;[20] in comparison, the world record for the smallest cross section of a successful reaction was 30 fb for the reaction 209Bi(70Zn,n)278Nh,[10] and Kratz predicted a maximum cross section of 20 fb for producing ununennium.[20] If these predictions are accurate, then synthesizing ununennium would be at the limits of current technology, and synthesizing unbinilium would require new methods.[20]

This reaction was investigated again in April to September 2012 at the GSI. This experiment used a 249Bk target and a 50Ti beam to produce element 119, but since 249Bk decays to 249Cf with a half-life of about 327 days, both elements 119 and 120 could be searched for simultaneously:

24997Bk + 5022Ti → 299119Uue* → no atoms
24998Cf + 5022Ti → 299120Ubn* → no atoms

Neither element 119 nor element 120 was observed. This implied a limiting cross section of 65 fb for producing element 119 in these reactions, and 200 fb for element 120.[21]

In May 2021, the JINR announced plans to investigate the 249Cf+50Ti reaction in their new facility.[22] The 249Cf target would have been produced by the Oak Ridge National Laboratory in Oak Ridge, Tennessee , United States; the 50Ti beam would be produced by the Hubert Curien Pluridisciplinary Institute in Strasbourg, Alsace, France.[23] However, after the Russian invasion of Ukraine began in 2022, collaboration between the JINR and other institutes completely ceased due to sanctions.[24] Thus, the JINR's plans have since shifted to the 248Cm+54Cr reaction, where the target and projectile beam could both be made in Russia.[23][25]

Starting from 2022,[26] plans began to be made to use the 88-inch cyclotron in the Lawrence Berkeley National Laboratory (LBNL) in Berkeley, California , United States to attempt to make new elements using 50Ti projectiles. The plan is to first test them on a plutonium target to create livermorium (element 116) in late 2023. If that is successful, an attempt to make element 120 in the 249Cf+50Ti reaction will begin, probably in 2024 at the earliest.[27][28]

References

  1. ↑ Isospin dependence in heavy-element synthesis in fusion-evaporation reactions with neutron-rich radioactive ion-beams, A. Yakushev et al.
  2. ↑ 2.0 2.1 "Superheavy Element Factory: overview of obtained results". Joint Institute for Nuclear Research. 24 August 2023. http://www.jinr.ru/posts/superheavy-element-factory-overview-of-obtained-results/. 
  3. ↑ 3.0 3.1 Hoffman, S. (2008). Probing shell effects at Z = 120 and N = 184 (Report). GSI Scientific Report. p. 131. 
  4. ↑ "A New Block on the Periodic Table". Lawrence Livermore National Laboratory. April 2007. https://www.llnl.gov/str/April07/pdfs/04_07.4.pdf. 
  5. ↑ Itkis, M. G.; Oganessian, Yu. Ts. (2007). "Synthesis of New Nuclei and Study of Nuclear Properties and Heavy-Ion Reaction Mechanisms". Joint Institute for Nuclear Research. http://wwwinfo.jinr.ru/plan/ptp-2007/e751004.htm. 
  6. ↑ 6.0 6.1 Oganessian, Yu. Ts. et al. (2009). "Attempt to produce element 120 in the 244Pu+58Fe reaction". Phys. Rev. C 79 (2): 024603. doi:10.1103/PhysRevC.79.024603. Bibcode: 2009PhRvC..79b4603O. 
  7. ↑ "New darmstadtium isotope discovered at Superheavy Element Factory". Joint Institute for Nuclear Research. 27 February 2023. http://www.jinr.ru/posts/new-darmstadtium-isotope-discovered-at-superheavy-element-factory/. 
  8. ↑ 8.0 8.1 Düllmann, C. E. (20 October 2011). "Superheavy Element Research: News from GSI and Mainz". http://www.yumpu.com/en/document/view/7293741/superheavy-element-research-superheavy-element-research. 
  9. ↑ GSI (5 April 2012). "Searching for the island of stability". GSI. https://www.gsi.de/de/work/forschung/nustarenna/nustarenna_divisions/she_physik/research/super_heavy_elements/future_projects.htm. 
  10. ↑ 10.0 10.1 Zagrebaev, Karpov & Greiner 2013.
  11. ↑ 11.0 11.1 Hofmann, S.; Heinz, S.; Mann, R. et al. (2016). "Review of even element super-heavy nuclei and search for element 120". The European Physical Journal A 2016 (52): 180. doi:10.1140/epja/i2016-16180-4. Bibcode: 2016EPJA...52..180H. https://www.researchgate.net/publication/304459935. 
  12. ↑ Hofmann, S.; Heinz, S.; Mann, R.; Maurer, J.; Münzenberg, G.; Antalic, S.; Barth, W.; Burkhard, H. G. et al. (2016). "Remarks on the Fission Barriers of SHN and Search for Element 120". in Peninozhkevich, Yu. E.; Sobolev, Yu. G.. Exotic Nuclei. pp. 155–164. ISBN 9789813226555. 
  13. ↑ Adcock, Colin (2 October 2015). "Weighty matters: Sigurd Hofmann on the heaviest of nuclei". Journal of Physics G: Nuclear and Particle Physics. https://jphysplus.iop.org/2015/10/02/weighty-matters-sigurd-hofmann-on-the-heaviest-of-nuclei/. 
  14. ↑ Hofmann, Sigurd (August 2015). "Search for Isotopes of Element 120 on the Island of SHN". Exotic Nuclei: 213–224. doi:10.1142/9789814699464_0023. ISBN 978-981-4699-45-7. Bibcode: 2015exon.conf..213H. 
  15. ↑ Heßberger, F. P.; Ackermann, D. (2017). "Some critical remarks on a sequence of events interpreted to possibly originate from a decay chain of an element 120 isotope". The European Physical Journal A 53 (123): 123. doi:10.1140/epja/i2017-12307-5. Bibcode: 2017EPJA...53..123H. 
  16. ↑ JINR (29 March 2022). "At seminar on synthesis of element 120". JINR. http://www.jinr.ru/posts/at-seminar-on-synthesis-of-element-120/. 
  17. ↑ Mayer, Anastasiya (31 May 2023). "«Большинство наших партнеров гораздо мудрее политиков»". Vedomosti. https://www.vedomosti.ru/technology/characters/2023/05/31/977789-bolshinstvo-nashih-partnerov-mudree-politikov. "В этом году мы фактически завершаем подготовительную серию экспериментов по отладке всех режимов ускорителя и масс-спектрометров для синтеза 120-го элемента. Научились получать высокие интенсивности ускоренного хрома и титана. Научились детектировать сверхтяжелые одиночные атомы в реакциях с минимальным сечением. Теперь ждем, когда закончится наработка материала для мишени на реакторах и сепараторах у наших партнеров в «Росатоме» и в США: кюрий, берклий, калифорний. Надеюсь, что в 2025 г. мы полноценно приступим к синтезу 120-го элемента." 
  18. ↑ 18.0 18.1 Yakushev, A. (2012). "Superheavy Element Research at TASCA". http://asrc.jaea.go.jp/soshiki/gr/chiba_gr/workshop3/&Yakushev.pdf. 
  19. ↑ Siwek-Wilczyńska, K.; Cap, T.; Wilczyński, J. (April 2010). "How can one synthesize the element Z = 120?". International Journal of Modern Physics E 19 (4): 500. doi:10.1142/S021830131001490X. Bibcode: 2010IJMPE..19..500S. 
  20. ↑ 20.0 20.1 20.2 Kratz, J. V. (5 September 2011). "The Impact of Superheavy Elements on the Chemical and Physical Sciences". 4th International Conference on the Chemistry and Physics of the Transactinide Elements. http://tan11.jinr.ru/pdf/06_Sep/S_1/02_Kratz.pdf. Retrieved 27 August 2013. 
  21. ↑ Khuyagbaatar, J.; Yakushev, A.; Düllmann, Ch. E. et al. (December 2020). "Search for elements 119 and 120". Physical Review C 102 (6): 064602. doi:10.1103/PhysRevC.102.064602. Bibcode: 2020PhRvC.102f4602K. https://jyx.jyu.fi/bitstream/handle/123456789/73027/2/khuyagbaatarym0812.pdf. Retrieved 25 January 2021. 
  22. ↑ Sokolova, Svetlana; Popeko, Andrei (24 May 2021). "How are new chemical elements born?". JINR. http://www.jinr.ru/posts/how-are-new-chemical-elements-born/. "Previously, we worked mainly with calcium. This is element 20 in the Periodic Table. It was used to bombard the target. And the heaviest element that can be used to make a target is californium, 98. Accordingly, 98 + 20 is 118. That is, to get element 120, we need to proceed to the next particle. This is most likely titanium: 22 + 98 = 120.

    There is still much work to adjust the system. I don’t want to get ahead of myself, but if we can successfully conduct all the model experiments, then the first experiments on the synthesis of element 120 will probably start this year."     
  23. ↑ 23.0 23.1 Riegert, Marion (19 July 2021). "In search of element 120 in the periodic table of elements". University of Strasbourg. https://en.unistra.fr/unistra-news/research/in-search-of-element-120-in-the-periodic-table-of-elements. 
  24. ↑ Ahuja, Anjana (18 October 2023). "Even the periodic table must bow to the reality of war". Financial Times. https://www.ft.com/content/6b6b0afc-39b2-4955-af5a-d0ea6b4d8306. 
  25. ↑ "В ЛЯР ОИЯИ впервые в мире синтезирован ливерморий-288" (in ru). Joint Institute for Nuclear Research. 23 October 2023. http://www.jinr.ru/posts/v-lyar-oiyai-vpervye-v-mire-sintezirovan-livermorij-288/. 
  26. ↑ Gates, J.; Pore, J.; Crawford, H.; Shaughnessy, D.; Stoyer, M. A. (25 October 2022). The Status and Ambitions of the US Heavy Element Program. doi:10.2172/1896856. https://www.osti.gov/servlets/purl/1896856. Retrieved 13 November 2022. 
  27. ↑ Chapman, Kit (10 October 2023). "Berkeley Lab to lead US hunt for element 120 after breakdown of collaboration with Russia". Chemistry World. https://www.chemistryworld.com/news/berkeley-lab-to-lead-us-hunt-for-element-120-after-breakdown-of-collaboration-with-russia/4018207.article. 
  28. ↑ Biron, Lauren (16 October 2023). "Berkeley Lab to Test New Approach to Making Superheavy Elements". Lawrence Berkeley National Laboratory. https://physicalsciences.lbl.gov/2023/10/16/berkeley-lab-to-test-new-approach-to-making-superheavy-elements/. 

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